Light changes of the close binary system CN Andromedae

Details Light changes of the close binary system CN Andromedae Light changes of the close binary system CN Andromedae

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..191k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 191-199.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Photometry, Eclipsing Binary Stars, Electrophotometry, Stellar Color, Stellar Spectrophotometry, Light Curve, Periodic Variations, Tables (Data), Visual Photometry

Scientific paper

The photoelectric B and V color observations of the Beta Lyrae-type eclipsing binary CN And were made on four nights at the Ege University Observatory. The new light elements, which were calculated by adding new times of minima obtained during the observations to the previous ones, were given. The light curve of the system varies cycle by cycle, and the variation is discussed in some extent.

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